Wide-angle giant photonic spin Hall effect
Photonic spin Hall effect is a manifestation of spin-orbit interaction of light and can be measured by a transverse shift \lambda of photons with opposite spins. The precise measurement of transverse shifts can enable many spin-related applications, such as precise metrology and optical sensing. Ho...
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sg-ntu-dr.10356-1642402023-02-28T20:08:51Z Wide-angle giant photonic spin Hall effect Chen, Zhihao Chen, Yu Wu, Yaodong Zhou, Xinxing Sun, Handong Low, Tony Chen, Hongsheng Lin, Xiao School of Physical and Mathematical Sciences Centre for Disruptive Photonic Technologies (CDPT) Science::Physics Epsilon-Near Zeros Free Spaces Photonic spin Hall effect is a manifestation of spin-orbit interaction of light and can be measured by a transverse shift \lambda of photons with opposite spins. The precise measurement of transverse shifts can enable many spin-related applications, such as precise metrology and optical sensing. However, this transverse shift is generally small (i.e. \delta /\lambda <{10}^{-1}, \lambda is the wavelength), which impedes its precise measurement. To-date proposals to generate giant spin Hall effect (namely with \delta /\lambda >{10}^{2}) have severe limitations, particularly its occurrence only over a narrow angular cone (with a width of \Delta \theta <{1}^{\circ}). Here we propose a universal scheme to realize the wide-angle giant photonic spin Hall effect with \Delta \theta >{70}^{\circ} by exploiting the interface between free space and uniaxial epsilon-near-zero media. The underlying mechanism is ascribed to the almost-perfect polarization splitting between s and p polarized waves at the designed interface. Remarkably, this almost-perfect polarization splitting does not resort to the interference effect and is insensitive to the incident angle, which then gives rise to the wide-angle giant photonic spin Hall effect. Ministry of Education (MOE) Published version X.L. was sponsored in part by the National Natural Science Foundation of China (62175212), the National Natural Science Fund for Excellent Young Scientists Fund Program (Overseas) of China, the Fundamental Research Funds for the Central Universities (2021FZZX001-19), and Zhejiang University Global Partnership Fund. X.Z. was supported by the National Natural Science Foundation of China (11604095). H.S. acknowledges support from the Singapore Ministry of Education AcRF Tier 1 [RG95/19 (S)]. 2023-01-11T02:30:52Z 2023-01-11T02:30:52Z 2022 Journal Article Chen, Z., Chen, Y., Wu, Y., Zhou, X., Sun, H., Low, T., Chen, H. & Lin, X. (2022). Wide-angle giant photonic spin Hall effect. Physical Review B, 106(7), 075409-1-075409-7. https://dx.doi.org/10.1103/PhysRevB.106.075409 1098-0121 https://hdl.handle.net/10356/164240 10.1103/PhysRevB.106.075409 2-s2.0-85136238435 7 106 075409-1 075409-7 en RG95/19 (S) Physical Review B ©2022 American Physical Society. All rights reserved. This paper was published in Physical Review B and is made available with permission of American Physical Society. application/pdf |
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Science::Physics Epsilon-Near Zeros Free Spaces Chen, Zhihao Chen, Yu Wu, Yaodong Zhou, Xinxing Sun, Handong Low, Tony Chen, Hongsheng Lin, Xiao Wide-angle giant photonic spin Hall effect |
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Photonic spin Hall effect is a manifestation of spin-orbit interaction of
light and can be measured by a transverse shift \lambda of photons with opposite spins. The precise measurement of transverse shifts can enable many spin-related applications, such as precise metrology and optical sensing. However, this transverse shift is generally small (i.e. \delta /\lambda <{10}^{-1}, \lambda is the wavelength), which impedes its precise measurement. To-date proposals to generate giant spin Hall effect (namely with \delta /\lambda >{10}^{2}) have severe limitations, particularly its occurrence only over a narrow angular cone (with a width of \Delta \theta <{1}^{\circ}). Here we propose a universal scheme to realize the wide-angle giant photonic spin Hall effect with \Delta \theta >{70}^{\circ} by exploiting the interface between free space and uniaxial epsilon-near-zero media. The underlying
mechanism is ascribed to the almost-perfect polarization splitting between s and p polarized waves at the designed interface. Remarkably, this almost-perfect polarization splitting does not resort to the interference effect and is insensitive to the incident angle, which then gives rise to the wide-angle giant photonic spin Hall effect. |
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School of Physical and Mathematical Sciences |
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School of Physical and Mathematical Sciences Chen, Zhihao Chen, Yu Wu, Yaodong Zhou, Xinxing Sun, Handong Low, Tony Chen, Hongsheng Lin, Xiao |
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Article |
author |
Chen, Zhihao Chen, Yu Wu, Yaodong Zhou, Xinxing Sun, Handong Low, Tony Chen, Hongsheng Lin, Xiao |
author_sort |
Chen, Zhihao |
title |
Wide-angle giant photonic spin Hall effect |
title_short |
Wide-angle giant photonic spin Hall effect |
title_full |
Wide-angle giant photonic spin Hall effect |
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Wide-angle giant photonic spin Hall effect |
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Wide-angle giant photonic spin Hall effect |
title_sort |
wide-angle giant photonic spin hall effect |
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2023 |
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https://hdl.handle.net/10356/164240 |
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1759855558395953152 |